2026-10-15T00:09:48Zhttps://docta.ucm.es/rest/oai/requestoai:docta.ucm.es:20.500.14352/63912023-08-04T02:28:25Zcom_20.500.14352_14col_20.500.14352_15
Docta Complutense
author
Danchev, I. C.
author
Antonov, A. N.
author
Kadrev, D. N.
author
Gaidarov, M. K.
author
Sarriguren, P.
author
Moya de Guerra, Elvira
2023-06-16T15:20:08Z
2023-06-16T15:20:08Z
2020-06-16
0556-2813
10.1103/PhysRevC.101.064315
https://hdl.handle.net/20.500.14352/6391
https://doi.org/10.1103/PhysRevC.101.064315
https://journals.aps.org/
We derive the values of nuclear symmetry energy, its components, as well as pressure in finite nuclei at saturation density from their corresponding values in nuclear matter obtained in nonrelativistic Brueckner-Hartree-Fock calculations with the realistic Bonn B and Bonn CD potentials using the coherent density fluctuation model in the framework of a self-consistent Skyrme-Hartree-Fock plus BCS method. We focus on three isotopic chains of spherical nuclei (Ni, Sn, and Pb) and compare our results with those obtained with an effective Brueckner density-dependent potential. The role of the three-body forces on the considered quantities is also studied and discussed.
eng
Symmetry energy properties of neutron-rich nuclei from the coherent density fluctuation model applied to nuclear matter calculations with Bonn potentials
journal article
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MoyadeGuerra05preprint.pdf
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MoyadeGuerra05preprint.pdf.txt